In astronomy, the term period usually refers to how long an object takes to complete one cycle of revolution. In particular the orbital period of a star or planet is the time it takes to return to the same place in the orbit. The spin period of a star is the time it takes to rotate on its axis. 

Alternately, a wave period is the time taken for one complete cycle of the wave to pass a reference point.
The period, P of an orbit, rotation, or wave, is just the inverse of the frequency, f:
The orbital period, P of two bodies of mass M and m that are gravitationally bound and separated by a distance R is:
Here G is Newton’s gravitational constant.
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